Emission of solar chromospheric and transition region features related to the underlying magnetic field

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Table 1.

IRIS data sets used in this study.

		Date	Start (UT)	End (UT)	Exposure time	Raster type^a	X^b	Y^c
Active region	(AR 11850)	24 Sep. 2013	11:44:43	12:04:10	2 s		−265″	+88″
Quiet Sun	(QS)	13 Oct. 2013	23:27:28	02:59:15 (+1d)	30 s	400 × 0.35″	−120″	−41″
Coronal hole	(CH)	12 Oct. 2013	12:20:28	15:52:15	30 s		+314″	−140″

Notes.

^(a)

In all cases large dense rasters were performed with a field-of-view of about 140″ × 170″. These required 400 raster steps of 0.35″ each in the east-west (solar-X) direction.

^(b)

The values for X and Y give the distance of the centre of the field-of-view from disc centre in the solar-X and Y directions.

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